NuSTAR detection of 4s Hard X-ray Lags from the Accreting Pulsar GS 0834-430

NuSTAR detection of 4s Hard X-ray Lags from the Accreting Pulsar GS 0834-430

The NuSTAR hard X-ray telescope observed the transient Be/X-ray binary GS 0834–430 during its 2012 outburst. The source is detected between 3 – 79 keV with high statistical significance, and we were able to perform very accurate spectral and timing analysis. The phase-averaged spectrum is consistent...

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Bibliographic Details
Main Authors: Bachetti, Matteo, Miyasaka, Hiromasa, Harrison, Fiona A., Furst, Felix, Barret, Didier, Bellm, Eric C., Boggs, Steven E., Chakrabarty, Deepto, Chenevez, Jerome, Christensen, Finn E., Craig, William W., Grefenstette, Brian W., Hailey, Charles J., Madsen, Kristin K., Natalucci, Lorenzo, Pottschmidt, Katja, Stern, Daniel, Tomsick, John A., Walton, Dominic J., Wilms, Jörn, Zhang, William
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: EDP Sciences 2014
Online Access:http://hdl.handle.net/1721.1/89218
https://orcid.org/0000-0001-8804-8946

Internet

http://hdl.handle.net/1721.1/89218
https://orcid.org/0000-0001-8804-8946

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